Astrophysics - Instrumentation and Methods for Astrophysics
Abstract :
[en] The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) dataset will dramatically alter our understanding of the Universe, from the origins of the Solar System to the nature of dark matter and dark energy. Much of this research will depend on the existence of robust, tested, and scalable algorithms, software, and services. Identifying and developing such tools ahead of time has the potential to significantly accelerate the delivery of early science from LSST. Developing these collaboratively, and making them broadly available, can enable more inclusive and equitable collaboration on LSST science. To facilitate such opportunities, a community workshop entitled "From Data to Software to Science with the Rubin Observatory LSST" was organized by the LSST Interdisciplinary Network for Collaboration and Computing (LINCC) and partners, and held at the Flatiron Institute in New York, March 28-30th 2022. The workshop included over 50 in-person attendees invited from over 300 applications. It identified seven key software areas of need: (i) scalable cross-matching and distributed joining of catalogs, (ii) robust photometric redshift determination, (iii) software for determination of selection functions, (iv) frameworks for scalable time-series analyses, (v) services for image access and reprocessing at scale, (vi) object image access (cutouts) and analysis at scale, and (vii) scalable job execution systems. This white paper summarizes the discussions of this workshop. It considers the motivating science use cases, identified cross-cutting algorithms, software, and services, their high-level technical specifications, and the principles of inclusive collaborations needed to develop them. We provide it as a useful roadmap of needs, as well as to spur action and collaboration between groups and individuals looking to develop reusable software for early LSST science.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Breivik, Katelyn
Connolly, Andrew J.
Ford, K. E. Saavik
Jurić, Mario
Mandelbaum, Rachel
Miller, Adam A.
Norman, Dara
Olsen, Knut
O'Mullane, William
Price-Whelan, Adrian
Sacco, Timothy
Sokoloski, J. L.
Villar, Ashley
Acquaviva, Viviana
Ahumada, Tomas
AlSayyad, Yusra
Alves, Catarina S.
Andreoni, Igor
Anguita, Timo
Best, Henry J.
Bianco, Federica B.
Bonito, Rosaria
Bradshaw, Andrew
Burke, Colin J.
Rodrigues de Campos, Andresa
Cantiello, Matteo
Caplar, Neven
Chandler, Colin Orion
Chan, James
Nicolaci da Costa, Luiz
Danieli, Shany
Davenport, James R. A.
Fabbian, Giulio
Fagin, Joshua
Gagliano, Alexander
Gall, Christa
Garavito Camargo, Nicolás
Gawiser, Eric
Gezari, Suvi
Gomboc, Andreja
Gonzalez-Morales, Alma X.
Graham, Matthew J.
Gschwend, Julia
Guy, Leanne P.
Holman, Matthew J.
Hsieh, Henry H.
Hundertmark, Markus
Ilić, Dragana
Ishida, Emille E. O.
Jurkić, Tomislav
Kannawadi, Arun
Kosakowski, Alekzander
Kovačević, Andjelka B.
Kubica, Jeremy
Lanusse, François
Lazar, Ilin
Levine, W. Garrett
Li, Xiaolong
Lu, Jing
Luna, Gerardo Juan Manuel
Mahabal, Ashish A.
Malz, Alex I.
Mao, Yao-Yuan
Medan, Ilija
Moeyens, Joachim
Nikolić, Mladen
Nikutta, Robert
O'Dowd, Matt
Olsen, Charlotte
Pearson, Sarah
Villicana Pedraza, Ilhuiyolitzin
Popinchalk, Mark
Popović, Luka C.
Pritchard, Tyler A.
Quint, Bruno C.
Radović, Viktor
Ragosta, Fabio
Riccio, Gabriele
Riley, Alexander H.
Rożek, Agata
Sánchez-Sáez, Paula
Sarro, Luis M.
Saunders, Clare
Savic, Djordje ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Space sciences, Technologies and Astrophysics Research (STAR) ; Astronomical Observatory of Belgrade, Serbia